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Berkeley 32: A Metal-poor and Dynamically Evolved Open Cluster with Evidence of Radial Migration

  • Authors: D. C. Çinar, D. Bisht, Ing-Guey Jiang, W. H. Elsanhoury, K. Belwal, Selçuk Bilir

D. C. Çinar et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

RDP and MCMC posterior distributions for Berkeley 32. Upper panel: observed surface density (ρ) as a function of radial distance from the cluster center (black points with Poisson error bars). The solid red curve is the best-fitting I. King (1962) model, with the shaded region indicating the 1σ confidence interval. The horizontal blue dashed line marks the background density level (ρbg). Lower panels: corner plot of the posterior distributions for the fitted King model parameters (ρ0, rc, rt, ρbg), with median values (solid red lines) and 1σ boundaries (dashed lines).

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